Interactive tools – Generate Input Files & Convert Parameters
Generate Input Files
Use the interactive tools below to generate custom .ini
configuration files by selecting your desired AO mode, instrument, and parameter values.
Select your AO mode to begin:
Conversion from Magnitude to Number of Photons per Subaperture per Frame
The value of the parameter NumberPhotons
in (expressed in photons per subaperture per frame) for a natural guide star
of a given magnitude is calculated using the following formula:
Parameter definitions
B band | V band | R band | I band | J band | H band | K band | |
---|---|---|---|---|---|---|---|
(Zero Point) | |||||||
Spectral band extinction correction
For a spectral class M0V star, the apparent magnitude is corrected by an extinction term that varies by band:
B band | V band | R band | I band | J band | H band | K band | |
---|---|---|---|---|---|---|---|
This formula converts the visual magnitude, corrected for spectral band extinction, into the expected number of photons detected per subaperture per frame. It takes into account instrumental parameters such as the telescope’s effective collecting area, the number of wavefront sensor lenslets, the total system throughput, and the wavefront sensor's frame rate.
Below is an interactive interface that allows you to calculate the NumberPhotons
TipTop parameter from a given magnitude for the selected instrument.
Conversion from Magnitude to Number of Photons
Number of lenslets: 40
Sensor frame rate: 1000 Hz